Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00568925" target="_blank" >RIV/67985815:_____/22:00568925 - isvavai.cz</a>
Alternative codes found
RIV/68378271:_____/22:00568845
Result on the web
<a href="https://pos.sissa.it/395/547/pdf" target="_blank" >https://pos.sissa.it/395/547/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.395.0547" target="_blank" >10.22323/1.395.0547</a>

Result language
angličtina
Original language name
Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre
Original language description
This talk will summarise the planned dark matter search strategies with CTA, focusing on the signal from the Galactic centre. As observed with the Fermi LAT at lower energies, this region is rather complex and CTA will be the first ground-based observatory sensitive to the large scale diffuse astrophysical emission from that region. We report on the collaboration effort to study thenimpact of such extended astrophysical backgrounds on the dark matter search, based on Fermi-LAT data in order to guide our observational strategies, taking into account various sources of systematic uncertainty.
Czech name
—
Czech description
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Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2022
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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